首页> 外文会议>Advanced Maui Optical and Space Surveillance Technologies Conference >Chimera: a high-speed three-color photometer for satellite characterization
【24h】

Chimera: a high-speed three-color photometer for satellite characterization

机译:嵌合体:用于卫星表征的高速三色光度计

获取原文

摘要

High-speed optical photometers have been used for decades to characterize man-made satellites and space debris in Earth orbit. In the 1970s and 1980s, these instruments were typically based on photomultiplier tubes (PMT) and provided single-color, or in some cases simultaneous multicolor, photometric data with high time resolution. The original GEODSS PMT photometers were designed to collect photometry on deep space satellites at rates up to 1 kHz. CCDs have since displaced the use of PMTs in photometers in the astronomical community and the GEODSS system. CCDs offer higher quantum efficiency and two-dimensional imaging arrays, but at a lower speed than PMTs. The latest developments and introductions of commercially available Electron-Multiplying CCD (EMCCD) imagers is driving a renaissance in this field with several new instruments in development. Chimera is a high-speed photometer with simultaneous three-color photometry in the Sloan r' (562-695 nm). i' (695-844). and z' (826-920 nm) bands. The optical design provides well-corrected fields of view of 9.7 arcmin in the z' band and 6.0 arcmin in r' and i' bands on the Steward Observatory 61" Kuiper telescope at Mt. Lemmon. The wide field of view facilitates acquisition and tracking of rapidly moving satellites and allows for a variety of photometric calibration methods. The optical design uses a wide-field collimator, two dichroic beam splitters, and three re-imagers. Chimera utilizes three Princeton Instruments Pro-EM HS cameras, which provide data at rates up to 228 Hz in full frame mode. Rates over 1000 Hz are possible by defining photometric regions of interest (ROIs). A highly-modified version of Michael Mommert's photometric pipeline (PP), originally developed for near-Earth asteroid photometry, is used for data processing. A real time graphical user interface is under development to allow real-time data quality assessment and period determination during data collections. In space surveillance, the optical sig
机译:已经使用了高速光学光度计数十年来描述地球轨道中的人造卫星和空间碎片。在20世纪70年代和20世纪80年代,这些仪器通常基于光电倍增管(PMT)并提供单色,或在某些情况下,具有高时间分辨率的同步多色的光度数据。原始地缘PMT光度计旨在在高达1 kHz的速率下收集在深空卫星上的光度测量。自从分离了天文社区和地理系统的光度计中的使用PMT以来,CCD具有。 CCD提供更高的量子效率和二维成像阵列,但速度低于PMTS。可商购电子 - 乘以CCD(EMCCD)成像仪的最新发展和介绍在这一领域推动了一个新的开发中的文艺复兴。嵌合体是一种高速光度计,在Sloan R'(562-695 nm)中具有同时三色度测光。我(695-844)。和z'(826-920 nm)频段。光学设计在Z'频段和6.0 arcmin中提供了良好的9.7 arcmin的视野,在r'和6.0 arcmin,我在Mt.Slemmon的管道望远镜上的R'和I'频段。宽阔的视野有助于获取和跟踪快速移动的卫星并允许各种光度校准方法。光学设计采用宽场准直器,两个二向色束分离器和三个重新成像。嵌合体利用三个普林斯顿仪器Pro-EM HS相机,它提供数据全帧模式中最多可达228赫兹。通过定义感兴趣的光度区域(ROI)来实现超过1000Hz的速率。最初为近地球小行星测光测量的Michael Mommert的光度管道(PP)的高度修改版本用于数据处理。正在开发的实时图形用户界面,以允许在数据收集期间实时数据质量评估和周期确定。在太空监控,光学信号

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号